4.8 Article

Exploring the Role of PAHs in the Formation of Soot: Pyrene Dimerization

期刊

JOURNAL OF PHYSICAL CHEMISTRY LETTERS
卷 1, 期 19, 页码 2962-2967

出版社

AMER CHEMICAL SOC
DOI: 10.1021/jz101033t

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资金

  1. French Programmes Physique Stellaire
  2. Physique et Chimie du Milieu Interstellaire
  3. Indo-French Centre for the Promotion of Advanced Research [3405-3]
  4. Region de Bretagne, Rennes Metropole
  5. European Union [MEXC-CT-2004-006734]
  6. NASA [NNH09AK241]
  7. U.S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences [DE-AC02-06CH11357]

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A critical step in currently accepted models for soot formation in combustion is the dimerization of polycyclic aromatic hydrocarbons as small as pyrene, which is necessary within these models to reproduce correctly the soot particle size distribution. We present experimental measurements on the kinetics of pyrene dimerization performed in low temperature supersonic flows with photoionization mass spectrometric detection, coupled with theoretical results based on careful consideration of the intermolecular interaction energies, binding energy, equilibrium constant, and intermolecular dynamics. These results demon strate that the equilibrium of the reaction strongly favors the dissociation of the pyrene dimer at high temperature and that physical dimerization (involving van der Waals forces) of pyrene cannot be a key step in carbon particle formation in hot environments such as flames and circumstellar shells.

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